PADC TAP Server on voparis-tap-sandbox.obspm.fr Public Tables

Result

Matched: 23

TablenameTableinfoTable desc.Res desc.
adityal1.epn_coreTable InfoN/A Spectroscopic observations of the solar corona with VELC is carried out in the emission line centred at 5303Å [Fe XIV]. This is also called the ‘green’ line. The pass band (Full Width at Half Maximum) of this spectroscopic channel is ~7Å. The field of view (FoV) covers the solar corona in the heliocentric distance range 1.05 - 1.5 solar radii (i.e. a height range of ~0.05 – 0.5 solar radii above the solar limb whose heliocentric distance is 1 solar radii). The radius of the occulting disk in the VELC is 1.05 solar radii. The pixel resolution for observations in the 5303 Å channel of VELC is 1.25 arcsec. Spectral dispersion is ~28mÅ.
apis.epn_coreTable InfoEpnCore table for APIS service Planetary aurorae are powerful emissions radiated from auroral regions of magnetized planets by accelerated charged particles, in a wide range of wavelengths (from radio to X-rays). The UV range in particular is adequate to measure collisionaly excited transitions of H and H2, the dominant species in the upper atmosphere of giant planets, produced by precipitating auroral particles, and benefits a good angular resolution. Auroral UV observations therefore provide a rich source of informations on planetary atmospheres and magnetospheres. They also offer a unique diagnostic to remotely probe the solar wind activity throughout the heliosphere.
csa.epn_coreTable InfoN/A The British Astronomical Association has been collecting observations since 1890. Here we provide access to Comet Observations, both visual and CCD. Informations for alternate target name come from caero resolver, and ephemeris from miriad, both services are from the coutesy og IMCCE-Observatoire de Paris-PSL
eso_test.epn_coreTable InfoESO solar system data Test of ingesting Solar System data from the ESO archive, 2nd part
ivoa.ObsCoreTable InfoThe IVOA-defined obscore table, containing generic metadata for datasets within this data centre.Definition and support code for the ObsCore data model and table.
lunar_craters.epn_coreTable InfoLunar crater catalogue This is the Moon Crater Database v1 by Salamunićcar et al, 2012, http://doi.org/10.1016/j.pss.2011.09.003 - an EPN-TAP version of their LU60645GT catalogue. The catalogues by McDowell, Rodionova, and Head have been integrated with the results of a Crater Shape-based interpolation crater detection algorithm and Lunar Orbiter Laser Altimeter (LOLA) data. This catalogue is globally complete up to ∼D≥8 km. The original version is distributed by USGS: https://astrogeology.usgs.gov/search/map/Moon/Research/Craters/GoranSalamuniccar_MoonCraters
mirs.epn_coreTable InfoN/A use fits image for authentication test using proprietary period in dachs
spectro_asteroids.epn_coreTable InfoN/A This service provides a compilation of spectra of asteroids in the visible and NIR range. It is composed of various libraries distributed as VizieR catalogues. Reformatted VOtable or fits versions are provided with thumbnails. Ephemeris data are retrieved from Miriade (IMCCE) for the reference date when possible.
spectro_planets.epn_coreTable InfoN/A This service provides a compilation of global spectra of planets and satellites in the visible and NIR range, for quick reference purpose. It is made from various libraries, including the Tohoku-Hiroshima-Nagoya Planet Spectra Library (Lundock et al 2009) and spectra from a USGS web site (R. Clark). Reformatted VOtable versions are provided together with links to the original data.
spectro_tno.epn_coreTable InfoEPN-TAP table for TNO and Centaur reflectance spectra Combined vis-nIR reflectance spectra of Trans-Neptunian Objects and Centaurs from Merlin et al. 2017 (A&A 604, A86). The spectra cover wavelengths from approximately 0.35 to 2.45 micron, normalized at 0.55 micron. Data were obtained with ESO/VLT instruments (FORS1, FORS2, ISAAC, SINFONI, XSHOOTER). This table includes 42 individual object spectra and 4 taxonomic mean spectra (BB, BR, IR, RR classes from the Barucci et al. 2005 taxonomy). Each row refers to a different spectrum provided in a separate file.
tap_schema.columnsTable InfoColumns in tables available for ADQL querying. PADC TAP Server on voparis-tap-sandbox.obspm.fr's Table Access Protocol (TAP) service with table metadata.
tap_schema.groupsTable InfoColumns that are part of groups within tables available for ADQL querying. PADC TAP Server on voparis-tap-sandbox.obspm.fr's Table Access Protocol (TAP) service with table metadata.
tap_schema.key_columnsTable InfoColumns participating in foreign key relationships between tables available for ADQL querying. PADC TAP Server on voparis-tap-sandbox.obspm.fr's Table Access Protocol (TAP) service with table metadata.
tap_schema.keysTable InfoForeign key relationships between tables available for ADQL querying. PADC TAP Server on voparis-tap-sandbox.obspm.fr's Table Access Protocol (TAP) service with table metadata.
tap_schema.schemasTable InfoSchemas containing tables available for ADQL querying. PADC TAP Server on voparis-tap-sandbox.obspm.fr's Table Access Protocol (TAP) service with table metadata.
tap_schema.tablesTable InfoTables available for ADQL querying. PADC TAP Server on voparis-tap-sandbox.obspm.fr's Table Access Protocol (TAP) service with table metadata.
terrestrial_impact_craters.epn_coreTable InfoTerrestrial Impact Craters This is an EPN-TAP version of the catalogue published by Kenkmann 2021, as distributed by the University of Freiburg: https://impact-craters.com/. This catalogue includes all known impact craters on Earth. The original version is available at https://onlinelibrary.wiley.com/doi/full/10.1111/maps.13657.
titan_profiles.epn_coreTable InfoEPNcore table for temperature, pressure and element abundance profiles in Titan's atmosphere. This database contains vertical profiles of temperature and composition in Titan's atmosphere at several altitudes below 750 km. These profiles were retrieved from the infrared spectra acquired by the Composite Infrared Spectrometer (CIRS) aboard the Cassini spacecraft. The retrieval method and the description of the used dataset are detailed by Vinatier et al. (2010), and completed in Mathé et al. (2020), and Vinatier et al. (2020). References ---------- - Vinatier et al. (**2010**) Analysis of Cassini/CIRS limb spectra of Titan acquired during the nominal mission: I. Hydrocarbons, nitriles and CO2 vertical mixing ratio profiles. *Icarus*, 206(2), 559-570. `doi:10.1016/j.icarus.2009.08.013 <https://doi.org/10.1016/j.icarus.2009.08.013>`_ - Mathé et al. (**2020**) Seasonal changes in the middle atmosphere of Titan from Cassini/CIRS observations: Temperature and trace species abundance profiles from 2004 to 2017. *Icarus*, 344, 113547. `doi:10.1016/j.icarus.2019.113547 <https://doi.org/10.1016/j.icarus.2019.113547>`_ - Vinatier et al. (**2020**), Temperature and chemical species distributions in the middle atmosphere observed during Titan's late northern spring to early summer. A&A 641, A116; `doi:10.1051/0004-6361/202038411 <https://doi.org/10.1051/0004-6361/202038411>`_
tmc.epn_coreTable InfoN/A Chandrayaan-2, India’s second mission to the Moon was launched by GSLV-MK-III in July 2019. Mission carries 13 scientific payloads on Orbiter. Orbiter is presently orbiting moon under 100km x 100 km circular orbit. The data collected from the instruments from the orbiter will be received, processed and archived in Indian Space Science Data Center (ISSDC) for dissemination and use by scientific community in India and abroad. The data from Chandrayaan-2 instruments should be archived in such a way that they are easily accessible by Internet through simple interfaces being used elsewhere for similar kind of missions. TMC-2 (Terrain Mapping Camera) is one of the scientific instrument hosted on the Chandrayaan-2 Orbiter. The instrument is passive electro-optical imaging camera operating in visible-panchromatic band (500-800nm), comprising three optical sensors Fore, Nadir and Aft placed with angles of +25 deg, 0 deg and -25 deg to have three stereo views of the same target as spacecraft moves along the track. PDS4 is the de facto international standard for long term archival of planetary science data.
tno_spectra.epn_coreTable InfoEPN-TAP table for TNO and Centaur reflectance spectra Combined vis-nIR reflectance spectra of Trans-Neptunian Objects and Centaurs from Merlin et al. 2017 (A&A 604, A86). The spectra cover wavelengths from approximately 0.35 to 2.45 micron, normalized at 0.55 micron. Data were obtained with ESO/VLT instruments (FORS1, FORS2, ISAAC, SINFONI, XSHOOTER). This table includes 42 individual object spectra and 4 taxonomic mean spectra (BB, BR, IR, RR classes from the Barucci et al. 2005 taxonomy). Each row refers to a different spectrum provided in a separate file.
ufe.mainTable InfoN/ATBD
vir_ros.epn_coreTable InfoSpectroscopy of comet 67P VIRTIS/Rosetta service: imaging spectroscopy of comet 67P in the visible and the near infrared. Assessment version from PI team database.
vros_geocor.epn_coreTable InfoSpectroscopy of comet 67P, recalibrated VIRTIS/Rosetta archive of radiometry and geometry corrected products, VIRTIS-M only. Completed with the PI team database.

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